oldsplit – Create a visibility subset from an existing visibility set – manipulation task
Description
T H I S T A S K I S D E P R E C A T E D I T W I L L B E R E M O V E D S O O N
Oldsplit is the general purpose program to make a new data set that is a subset or averaged form of an existing data set. General selection parameters are included, and one or all of the various data columns (DATA, LAG_DATA and/or FLOAT_DATA, and possibly MODEL_DATA and/or CORRECTED_DATA) can be selected.
Oldsplit is often used after the initial calibration of the data to make a smaller measurement set with only the data that will be used in further flagging, imaging and/or self-calibration. Oldsplit can average over frequency (channels) and time (integrations).
Parameters
Parameter |
Default |
Description |
|---|---|---|
vis |
|
|
outputvis |
|
|
datacolumn |
|
|
field |
|
|
spw |
|
|
width |
|
|
antenna |
|
|
timebin |
|
|
timerange |
|
|
scan |
|
|
intent |
|
|
array |
|
|
uvrange |
|
|
correlation |
|
|
observation |
|
|
combine |
|
|
keepflags |
|
|
keepmms |
|
Parameter Explanations
vis
''
Name of input measurement set
outputvis
''
Name of output measurement set
datacolumn
'corrected'
Which data column(s) to Oldsplit out
field
''
Select field using ID(s) or name(s)
spw
''
Select spectral window/channels
width
int(1)
Number of channels to average to form one output channel
antenna
''
Select data based on antenna/baseline
timebin
'0s'
Bin width for time averaging
timerange
''
Select data by time range
scan
''
Select data by scan numbers
intent
''
Select data by scan intents
array
''
Select (sub)array(s) by array ID number
uvrange
''
Select data by baseline length
correlation
''
Select correlations
observation
''
Select by observation ID(s)
combine
''
Let time bins span changes in scan and/or state
keepflags
True
If practical, keep completely flagged rows instead of dropping them.
keepmms
False
If the input is a multi-MS, make the output one, too. (experimental)